Heavy deformed nuclei in the shell model Monte Carlo method

dc.creatorAlhassid, Y.
dc.creatorFang, L.
dc.creatorNakada, H.
dc.date2007-10-09
dc.date.accessioned2026-07-07T11:53:27Z
dc.date.available2026-07-07T11:53:27Z
dc.descriptionWe extend the shell model Monte Carlo approach to heavy deformed nuclei using a new proton-neutron formalism. The low excitation energies of such nuclei necessitate calculations at low temperatures for which a stabilization method is implemented in the canonical ensemble. We apply the method to study a well deformed rare-earth nucleus, 162Dy. The single-particle model space includes the 50-82 shell plus 1f_{7/2} orbital for protons and the 82-126 shell plus 0h_{11/2}, 1g_{9/2} orbitals for neutrons. We show that the spherical shell model reproduces well the rotational character of 162Dy within this model space. We also calculate the level density of 162Dy and find it to be in excellent agreement with the experimental level density, which we extract from several experiments.
dc.description4 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/0710.1656
dc.identifierhttp://arxiv.org/abs/0710.1656
dc.identifierPhys.Rev.Lett.101:082501,2008
dc.identifierdoi:10.1103/PhysRevLett.101.082501
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/204542
dc.subjectNuclear Theory
dc.titleHeavy deformed nuclei in the shell model Monte Carlo method
dc.typetext

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